Science-advisor
REGISTER info/FAQ
Login
username
password
     
forgot password?
register here
 
Research articles
  search articles
  reviews guidelines
  reviews
  articles index
My Pages
my alerts
  my messages
  my reviews
  my favorites
 
 
Stat
Members: 3645
Articles: 2'504'928
Articles rated: 2609

26 April 2024
 
  » arxiv » astro-ph/0404554

 Article overview



Quakes in Solid Quark Stars
A. Z. Zhou ; R. X. Xu ; X. J. Wu ; N. Wang ; X. Y. Hong ;
Date 28 Apr 2004
Journal Astropart.Phys. 22 (2004) 73-79
Subject astro-ph hep-ph
AffiliationCAS), R. X. Xu (PKU), X. J. Wu (PKU), N. Wang (CAS), and X. Y. Hong (CAS
AbstractA starquake mechanism for pulsar glitches is developed in the solid quark star model. It is found that the general glitch natures (i.e., the glitch amplitudes and the time intervals) could be reproduced if solid quark matter, with high baryon density but low temperature, has properties of shear modulus mu = 10^{30~34} erg/cm^3 and critical stress sigma_c = 10^{18~24} erg/cm^3. The post-glitch behavior may represent a kind of damped oscillations.
Source arXiv, astro-ph/0404554
Services Forum | Review | PDF | Favorites   
 
Visitor rating: did you like this article? no 1   2   3   4   5   yes

No review found.
 Did you like this article?

This article or document is ...
important:
of broad interest:
readable:
new:
correct:
Global appreciation:

  Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.

browser Mozilla/5.0 AppleWebKit/537.36 (KHTML, like Gecko; compatible; ClaudeBot/1.0; +claudebot@anthropic.com)






ScienXe.org
» my Online CV
» Free


News, job offers and information for researchers and scientists:
home  |  contact  |  terms of use  |  sitemap
Copyright © 2005-2024 - Scimetrica